Recently it has been speculated that a set of diffeomorphisms exist which act
non-trivially on the horizon of some black holes such as kerr and Kerr-Newman
black hole. \cite{Haco:2018ske,Haco:2019ggi}. Using this symmetry in covariant
phase space formalism one can obtains conserved charges as surface integrals on
the horizon. Kerr-Bolt spacetime is well-known for its asymptotically topology
and has been studied widely in recent years. In this work we are going to study
Kerr-Bolt black hole and provide a holographically describtion of it in term of
warped confromal field theory.Comment: 10 page